Entropy functions for accelerating black holes
Andrea Boido, Jerome P. Gauntlett, Dario Martelli, James Sparks

TL;DR
This paper develops an entropy function for supersymmetric accelerating black holes in AdS4, enabling entropy computation without explicit solutions, and predicts dual holographic microstate counting via partition functions of Chern-Simons-matter theories.
Contribution
Introduces a novel entropy function for accelerating black holes in AdS4 that uplift to M-theory, facilitating entropy calculations without explicit solutions.
Findings
Entropy function for supersymmetric accelerating black holes in AdS4
Prediction of holographic microstate counting through partition functions
Framework for computing black hole entropy without explicit solutions
Abstract
We introduce an entropy function for supersymmetric accelerating black holes in , that uplift on general Sasaki-Einstein manifolds to solutions of M-theory. This allows one to compute the black hole entropy without knowing the explicit solutions. A dual holographic microstate counting would follow from computing certain supersymmetric partition functions of Chern-Simons-matter theories compactified on a spindle. We make a general prediction for a class of such partition functions in terms of ``blocks'', with each block being constructed from the partition function on a three-sphere.
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Cosmology and Gravitation Theories · Geometric Analysis and Curvature Flows
